The big multipolar group crossed the Sun disc since 27.08 to 9.09.01 along the mid latitudes of the Northern hemisphere. The most sunspot had powerful penumbra and nearby fine satellite with penumbra which were settled to the North from the main group's part. The Southern group's part consisted of two nearby sunspots with general penumbra which had "figure-of-eight", and fine sunspots behind it. The tail group's part was formed by the sunspot with perceptible sunspot and fine sunspots neighbouring it. In the first days a chain of fine sunspots was observed to the North from the tail sunspot. Neighbouring the central meridian the total region's area exceeded 700 m.s.h., and it was counted 50-60 sunspots in the group.
The fine sunspot with symmetrical penumbra was observed at the low latitudes of the Southern hemisphere since 1.09 to 7.09.01, in the Eastern part of the Sun disc.
The fast development of a bipolar region was observed at the mid latitudes of the Southern hemisphere since 3.09 to 13.09.01. The bipole consisted of the developed head sunspot with oblong penumbra and many small sunspots and pores which built "kaleidoscopic" combinations behind the main sunspots. In the evolution's peak the total region's area reached 300 m.s.h., and it was counted more 30 sunspots in the group.
The crumbled chain crossed the Sun disc since 4.09 to 15.09.01 along the mid latitudes of the Southern hemisphere. The central sunspot was the most developed and stable part of the group. The total region's area reached 300 m.s.h., and it was counted more 30 sunspots in the group.
The long chain of developed sunspots crossed the Sun disc since 5.09 to 18.09.01 along the 26th parallel of the Southern hemisphere. The maximal total area of the multipole reached 1200 m.s.h., and it was counted more 60 sunspots in the group. The most developed sunspot with complex penumbra was settled in the central part of the group, and rest sunspots had decay's state.
The big multipolar group crossed the Sun disc since 6.09 to 18.09.01 along the mid latitudes of the Southern hemisphere. The multipole consisted of the head sunspot with powerful oblong penumbra and a chain of many growing sunspots with penumbraes. Neighbouring the central meridian a growing sunspot with asymmetrical penumbra emerged in the forward chain's part which began moved to the North from the head sunspot, and the rest chain's part began decay. In the evolution's peak the total region's area exceeded 600 m.s.h., and it was counted more 50 sunspots in the group.
The growing bipolar group was observed at the tenth parallel of the Northern hemisphere since 7.09 to 12.09.01, in the Western part of the Sun disc. In the first days the bipole consisted of the small double sunspot with oblong penumbra and fine sunspot's chain. In next days the head sunspots began extend and divide, and the chain transformed into tail sunspots with developed penumbraes. Before set for the limb the total region's area reached 400 m.s.h.
The small bipolar group crossed the Sun disc since 6.09 to 16.09.01 along the high latitudes of the Northern hemisphere. From time to time the total bipole's area reached 100 m.s.h.
The big bipolar group was decaying at the mid latitudes of the Southern hemisphere since 11.09 to 24.09.01. In the first days the total region's area exceeded 300 m.s.h., and it was counted 20-25 sunspots in the group. The group consisted of the big head sunspot with asymmetrical penumbra and a long string of small sunspots and pores.
The bipolar group's decay was observed at the tenth parallel of the Northern hemisphere since 12.09 to 19.09.01, in the Eastern part of the Sun disc. In the first days the total region's area reached 150 m.s.h.
The fine bipolar group was observed at the mid latitudes of the Northern hemisphere since 13.09 to 21.09.01. The head sunspot had symmetrical penumbra.
The decaying sunspot with asymmetrical penumbra crossed the Sun disc since 16.09 to 28.09.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 300 m.s.h.
The perceptible sunspot with asymmetrical penumbra adjoyned to the bipolar region 09620 from the East since 16.09 to 28.09.01. The total region's area reached 200 m.s.h.
The growing bipolar group crossed the Sun disc since 16.09 to 26.09.01 along the mid latitudes of the Northern hemisphere. Before set for the limb the total region's area reached 300 m.s.h., moreover the tail sunspot turned out the very developed part of the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 17.09 to 29.09.01 along the equator. The total region's area reached 100 m.s.h.
The fine bipolar formation was observed at the 25th parallel of the Northern hemisphere since 18.09 to 22.09.01, to the East from the central meridian.
The small sunspot with penumbra crossed the Sun disc since 18.09 to 27.09.01 along the equator. After intersection of the central meridian several pore's fibres appeared at the sunspot's place which formed triangle form. The total region's area did not reach 100 m.s.h. even but in the same time it was counted more fifteen sunspots in the group.
The large multipole crossed the Sun disc since 18.09 to 1.10.01 along the mid latitudes of the Southern hemisphere. The group consisted of many big and small sunspots which were solid adjoyned but occupied considerable parallel's lenght. The total region's area reached 1000 m.s.h., and it was counted more 50 sunspots in the group.
The large sunspot with complex asymmetrical penumbra crossed the Sun disc since 20.09 to 2.10.01 along the high latitudes of the Southern hemisphere. Many fine umbra's pieces were embedded into the penumbra, and fine sunspots and pores appeared and disappeared neighbouring the penumbra. From time to time the total region's area reached 800 m.s.h., and it was counted 20-25 sunspots in the group.
The small sunspot with symmetrical penumbra crossed the Sun disc since 22.09 to 4.10.01 along the 23rd parallel of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
The perceptible bipolar group crossed the Sun disc since 22.09 to 4.10.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of fine sunspot's chain, and the tail sunspot had developed penumbra. From time to time the total region's area exceeded 100 m.s.h.
The fine bipolar group was observed at the high latitudes of the Noorthern hemisphere since 23.09 to 1.10.01. The head sunspot had symmetrical penumbra.
The spreading bipolar group crossed the Sun disc since 24.09 to 6.10.01 along the mid latitudes of the Northern hemisphere. The maximal total area exceeded 400 m.s.h., and it was counted 25-30 sunspots in the group. The most developed sunspot had symmetrical penumbra and was situated in the tail part of the group.
The opened bipolar group crossed the Sun disc since 24.09 to 6.10.01 along the mid latitudes of the Southern hemisphere. The fine head sunspot had symmetrical penumbra. The tail sunspot was larger and had symmetrical penumbra also. Fine sunspots and pores were observed neighbouring the tail sunspot. In the first days the total region's area reached 250 m.s.h.
The fine bipolar group crossed the Sun disc since 26.09 to 4.10.01 along the low latitudes of the Northern hemisphere. The head sunspot had symmetrical penumbra.
The perceptible bipolar group crossed the Sun disc since 27.09 to 9.10.01 along the mid latitudes of the Southern hemisphere. The bipole consisted of the big sunspott with asymmetrical penumbra and string of fine sunspots and pores behind it. The total region's area reached 200 m.s.h.
The insignificant bipolar group was settled at the high latitudes of the Northern hemisphere since 1.10 to 4.10.01. The tail sunspot had symmetrical penumbra.
The growing bipolar group was observed at the mid latitudes of the Southern hemisphere since 1.10 to 8.10.01, in the Western part of the Sun disc. Before set for the limb the total region area reached 200 m.s.h.
The small sunspot with symmetrical penumbra was observed at the low latitudes of the Southern hemisphere since 2.10 to 12.10.01. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. In the first days the total sunspot's area reached 100 m.s.h. The sunspot was slowly diminishing.
The decaying bipolar sunspots crossed the Sun disc since 3.10 to 13.10.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
The insignificant bipolar sunspots were observed at the high latitudes of the Northern hemisphere since 4.10 to 7.10.01, neighbouring the central meridian.
The nearby sunspots with developed symmetrical penumbraes crossed the Sun disc since 4.10 to 15.10.01 along the high latitudes of the Southern hemisphere. In the first days the total region's area reached 300 m.s.h.
The small bipolar group was observed at the high latitudes of the Southern hemisphere since 6.10 to 14.10.01. The tail sunspot had perceptible symmetrical penumbra. In the first days the total bipole's area reached 200 m.s.h.
The fine sunspot with symmetrical penumbra was observed at the high latitudes of the Northern hemisphere since 8.10 to 14.10.01, in the Eastern part of the Sun disc. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The opened bipolar group crossed the Sun disc since 9.10 to 21.10.01 along the mid latitudes of the Southern hemisphere. The bipole consisted of small sunspots with penumbraes which were parted by considerable longitude's distance. The total region's area reached 200 m.s.h.
The big bipolar group crossed the Sun disc since 10.10 to 23.10.01 along the mid latitudes of the Northern hemisphere. The bipole consisted of powerful sunspots with penumbraes, and space between the head and the tail parts of the group was almost free for sunspots. From time to time the total region's area exceeded 800 m.s.h.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 14.10 to 24.10.01 along the high latitudes of the Northern hemisphere. Pores of opposite magnetic polarity appeared and disappeared neighbouring the sunspot.
The curved sunspot's chain crossed the Sun disc since 15.10 to 26.10.01 along the mid latitudes of the Northern hemisphere. The total region's area reached 200 m.s.h., and it was counted 20-25 sunspots in the group.
The perceptible sunspot with oblong penumbra crossed the Sun disc since 16.10 to 28.10.01 along the mid latitudes of the Southern hemisphere. The sunspot was gradually bifurcated. The maximal total area of the region reached 500 m.s.h.
The crowded congestion of developed sunspots crossed the Sun disc since 17.10 to 30.10.01 along the high latitudes of the Southern hemisphere. The total region's area reached 550 m.s.h.
The perceptible sunspot with asymmetrical penumbra crossed the Sun disc since 18.10 to 30.10.01 along the equator. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot. The total region's area reached 150 m.s.h.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 20.10 to 31.10.01 along the low latitudes of the Northern hemisphere. From time to time pores of opposite magnetic polarity were observed neighbouring the sunspot.
The big multipolar group crossed the Sun disc since 23.10 to 2.11.01 along the low latitudes of the Northern hemisphere. The head part of the group consisted of double sunspot with powerful penumbra. The tail sunspot's congestion with general penumbra was continuously changing the form. The total region's area reached 700 m.s.h., and it was counted 40-50 sunspots in the group.
The small group was observed at the 24th parallel of the Southern hemisphere since 25.10 to 31.10.01, in the Western part of the Sun disc. The main sunspot had stable symmetrical penumbra.
The large multipolar group crossed the Sun disc since 25.10 to 6.11.01 along the mid latitudes of the Northern hemisphere. The multipole consisted of many developed sunspots with jagged penumbra. The group was continuously changing the contours. In the evolution's peak the total region's area reached 1200 m.s.h., and it was counted 60-65 sunspots in the group.
The large sunspot with penumbra crossed the Sun disc since 27.10 to 8.11.01 along the low latitudes of the Northern hemisphere. Small sunspots and pores of opposite magnetic polarity appeared and disappeared neighbouring the sunspot. From time to time the total region's area reached 600 m.s.h., and it was counted 25-30 sunspots in the group.
The bipolar chain of small sunspots crossed the Sun disc since 1.11 to 11.11.01 along the low latitudes of the Northern hemisphere. From time to time the total region's area exceeded 100 m.s.h., and it was counted 15-20 sunspots in the group.
The long chain of small sunspots and pores crossed the Sun disc since 1.11 to 13.11.01 along the high latitudes of the Southern hemisphere. The group was gradually decaying into three sunspot's clusters, and than it was slowly melting away the Sun disc's background. From time to time the total region's area exceeded 400 m.s.h., and it was counted 40-45 sunspots in the group.
The bipolar combination of several fine sunspots were parted by considerable longitude's distance. The group was observed at the 26th parallel of the Northern hemisphere since 3.11 to 13.11.01.
The fast development of the bipolar region was observed at the 27th parallel of the Southern hemisphere since 4.11 to 11.11.01. In the evolution's peak the total region's area reached 150 m.s.h., and it was counted 15-20 sunspots in the group.
The long multipolar group crossed the Sun disc since 4.11 to 18.11.01 along the mid latitudes of the Southern hemisphere. The head part of the group consisted of several developed sunspots with penumbraes which were gradually lining. The tail part of the group formed of several developed sunspots with general penumbra which were slowly stretching. Many fine sunspots and pores were settled between the big sunspots. Neighbouring the central meridian the multipole assumed closed magnetic configuration, the total region's area reached 1400 m.s.h., and it was counted more 60 sunspots in the group.
The perceptible sunspot with symmetrical penumbra crossed the Sun disc since 6.11 to 19.11.01 along the low latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
The quick-growing bipolar group was observed at the low latitudes of the Northern hemisphere since 7.11 to 13.11.02, in the Western part of the Sun disc. The head and the tail parts of the group extended in several times. Before set for the limb the total region's area reached 500 m.s.h.
The fine sunspot with symmetrical penumbra crossed the Sun disc since 7.11 to 20.11.01 along the mid latitudes of the Northern hemisphere. In the first days the total region's area reached 100 m.s.h.
The small sunspot with symmetrical penumbra crossed the Sun disc since 10.11 to 22.11.01 along the mid latitudes of the Northern hemisphere. From time to time the total region's area reached 100 m.s.h.
The large sunspot with asymmetrical penumbra crossed the Sun disc since 11.11 to 24.11.01 along the mid latitudes of the Northern hemisphere. Many fine sunspots and pores of opposite magnetic polarity were observed to the North from the sunspot. In the evolution's peak the total region's area reached 400 m.s.h., and it was counted 20-25 sunspots in the group.
The small bipolar group crossed the Sun disc since 12.11 to 24.11.01 along the 24th parallel of the Southern hemisphere. The bipole was oriented to the meridian. The Southern sunspot had symmetrical penumbra. In time the Northern sunspot had decayed. The total region's area reached 100-150 m.s.h.
